Super-inflation, non-singular bounce, and low multipoles

被引：44

作者：

Biswas, Tirthabir ^{[1
]}

Mazumdar, Anupam ^{[2
]}

机构：

[1] Loyola Univ, Dept Phys, New Orleans, LA 70118 USA

[2] Univ Lancaster, Consortium Fundamental Phys, Lancaster LA1 4YB, England

来源：

CLASSICAL AND QUANTUM GRAVITY | 2014年 / 31卷 / 02期

关键词：

super-inflation; bounce; low multipole anomaly; UNIVERSE;

D O I：

10.1088/0264-9381/31/2/025019

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In this paper we present a simple argument that shows a non-singular bouncing cosmology naturally yields an era of super-inflation which can precede the phase of normal potential driven inflation. One of the consequences of a super-inflation phase is that it might be able to account for suppressing the low multipole in the amplitude of the cosmic microwave background radiation. We estimate that the number of e-folds of super-inflation required to explain the current Planck data to be roughly three e-folds.

引用

页数：7

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